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| || '''[[LCGT|PROJECT TOP]]''' ||[[LCGT/subgroup/analysis|GW Analysis]] ||[[LCGT/subgroup/ifo|Interferometer]] ||[[LCGT/subgroup/vacuum|Vacuum & Cryostat]] ||[[LCGT/subgroup/laser|Laser & Optics]] ||[[LCGT/subgroup/machanics|Seismic Isolator]] ||[[LCGT/subgroup/infra|Infrastructure]] || |
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| * [[KAGRA/Subgroups/DAS/Meeting/Analysis2010|作業中ファイル(2010)]] |
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| * Estimated events for NS binary coalescence | * [[attachment:ns_event_estimation.pdf|Estimated number of events for NS binary coalescence]] |
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| * [[LCGT/Meeting/Analysis090519|2009-05-19]] | === 作業班 === * [[KAGRA/Subgroups/DAS/Meeting/Analysis090519|2009-05-19]] * [[KAGRA/Subgroups/DAS/Meeting/Analysis090427|2009-04-27]] |
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| * [[LCGT/Meeting/Analysis090427|2009-04-27]] | === 解析ミーティング === * [[KAGRA/Subgroups/DAS/Meeting/Analysis2010|2010]] * [[KAGRA/Subgroups/DAS/Meeting/Analysis2009|2009]] |
目的
世界初の重力波信号の直接検出に最大限貢献することを目指す。
初検出後は、重力波天文学の創生に寄与することが LCGT project の目標である。
Main Target among GW sources
連星中性子合体からの重力波を年数回程度観測すること。
Conceptual design
Preliminary design
Data Analysis White Paper 2009
Ref: LIGO document No. T080278-00 Table of Contents / LSC-Virgo white paper -DRAFT
- List of minimul analysis processes
- Procuderes for the first detection ant its confirmation
- Software developments
- Infrastructure for Data Analysis
Detailed design
Meeting
作業班